概括
铁石年龄揭示了它们母体的快速冷却,IIA铁在太阳系形成的1亿年内凝固. 其他铁石群体显示后来的冷却历史.
科学领域:
- 太空化学 太空化学
- 行星科学 行星科学
- 地质时间学 (Geochronology)
背景情况:
- 铁石提供了对早期太阳系过程的关键见解.
- 了解它们的形成和冷却年龄有助于限制行星进化时间表.
研究的目的:
- 为了确定铁石的- (Re-Os) 年龄和同位素组成.
- 为不同的铁石群建立精确的形成和冷却时间表.
主要方法:
- 使用了负热电离质谱法 (NTIMS).
- 分析的重点是和的度和的同位素组成.
主要成果:
- IIA铁石的同位素年龄大约为4.5亿年,不确定性为+/-31亿年.
- 对IIA铁石的最低允许年龄为4.46亿年.
- 其他铁石群在IIA同位周期上方绘制图案,暗示了后来的冷却.
结论:
- IIAB岩铁的母体融化和冷却速度很快,在100万年内形成了地铁.
- 与IIA石相比,其他铁石群体的行星体可能经历了较为晚的冷却阶段.
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